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Nature (London), 2024, Vol.626 (8000), p.737-741
2024
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Autor(en) / Beteiligte
Titel
JWST detection of heavy neutron capture elements in a compact object merger
Ist Teil von
  • Nature (London), 2024, Vol.626 (8000), p.737-741
Ort / Verlag
Nature Publishing Group
Erscheinungsjahr
2024
Beschreibungen/Notizen
  • The mergers of binary compact objects such as neutron stars and black holes are of central interest to several areas of astrophysics, including as the progenitors of gamma-ray bursts (GRBs), sources of high-frequency gravitational waves and likely production sites for heavy element nucleosynthesis via rapid neutron capture (the r-process). These heavy elements include some of great geophysical, biological and cultural importance, such as thorium, iodine and gold. Here we present observations of the exceptionally bright gamma-ray burst GRB 230307A. We show that GRB 230307A belongs to the class of long-duration gamma-ray bursts associated with compact object mergers, and contains a kilonova similar to AT2017gfo, associated with the gravitational-wave merger GW170817. We obtained James Webb Space Telescope mid-infrared (mid-IR) imaging and spectroscopy 29 and 61 days after the burst. The spectroscopy shows an emission line at 2.15 microns which we interpret as tellurium (atomic mass A=130), and a very red source, emitting most of its light in the mid-IR due to the production of lanthanides. These observations demonstrate that nucleosynthesis in GRBs can create r-process elements across a broad atomic mass range and play a central role in heavy element nucleosynthesis across the Universe.
Sprache
Englisch
Identifikatoren
ISSN: 0028-0836
eISSN: 1476-4687
DOI: 10.1038/s41586-023-06759-1
Titel-ID: cdi_hal_primary_oai_HAL_hal_04170764v1
Format
Schlagworte
Astrophysics, Physics

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